Paper
10 August 1988 Anew High Speed Two-Dimensional Ccd Atmospheric Turbulence Monitor
A Howard Waldie, David B Soules, James J Drexler, Frank D Eaton, William A Peterson, John R Hines
Author Affiliations +
Abstract
A new atmospheric turbulence monitor utilizes relative motion between dual images of a single star, formed by two subapertures of a Schmidt-Cassegrain telescope, to calculate Fried's atmospheric seeing parameter, r0. Dual images are formed on a two-dimensional CCD array, and intensity at each pixel location is digitized for calculations by the host computer. Flexibility in frame rate, exposure time, and data processing are incorporated into the system design through extensive use of programmable array logic, state machines, and microcomputer control. The equipment eliminates many problems characteristic of current systems which use one-dimensional detectors and a single image.
© (1988) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
A Howard Waldie, David B Soules, James J Drexler, Frank D Eaton, William A Peterson, and John R Hines "Anew High Speed Two-Dimensional Ccd Atmospheric Turbulence Monitor", Proc. SPIE 0926, Optical, Infrared, Millimeter Wave Propagation Engineering, (10 August 1988); https://doi.org/10.1117/12.945792
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Frame grabbers

Telescopes

Clocks

Sensors

Extremely high frequency

Infrared radiation

Stars

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